A new study led by Keiichi Ohnaka, a researcher at Catholic University of the North in Chile, sought to understand how the distant
red supergiant star Antares manages to expel so much matter off its surface as it nears the end of its life and nears its finale as a spectacular supernova.
Antares is
a red supergiant star, and its large size makes it an ideal candidate for study from Earth.
Thorne has carried out a wide range of theoretical research in gravitation and astrophysics, including having predicted the existence of a type of
red supergiant star with a neutron star core, and using general relativity to describe how black holes move and precess.
Using ESO's Very Large Telescope Interferometer astronomers have constructed the most detailed image ever of a star —
the red supergiant star Antares.
A striking example can be seen in the constellation Orion, the hunter: his right shoulder is
the red supergiant star Betelgeuse and his left knee, the blue supergiant Rigel.
This picture of the dramatic nebula around the bright
red supergiant star Betelgeuse was created from images taken with the VISIR infrared camera on ESO's Very Large Telescope (VLT).
The Zoomable Universe: An Epic Tour Through Cosmic Scale, From Almost Everything to Nearly Nothing By Caleb Scharf What do a common cold - causing virus, an adult blue whale and
the red supergiant star Betelgeuse have in common?
In a study published in Solar and Stellar Astrophysics, the researchers say they saw
the red supergiant star N6946 - BH1 flare a million times brighter than our sun for several months in 2009 before fading out of visible wavelengths, a likely sign of a brand - new black hole.
Hubble has caught
a red supergiant star flaring up and disappearing — probably because it was transformed into a black hole
It's a shame they couldn't get along: each pattern is outlined by hot blue suns, and each boasts one of the sky's only two bright
red supergiant stars — Betelgeuse in Orion, and Antares, the heart of Scorpius.
The team calculated light curves of metal - poor supernova, produced by blue supergiant stars, and «metal - rich»
red supergiant stars.
Earlier sharp images have shown details on much more massive,
red supergiant stars like Betelgeuse and Antares.
Interacting supernovae from photoionization - confined shells around
red supergiant stars.
The new picture of Betelgeuse's atmosphere also helps resolve the mystery of how massive amounts of dust and gas are expelled from
red supergiant stars, an important source of enrichment for the interstellar medium.
Fine details show throughout the galaxy's arms, disk, bulge, and nucleus - blue and
red supergiant stars, star clusters, and star - forming regions, and dust lanes trace out fine structures in the disk and bar.
Not exact matches
Before 1987A, astronomers thought that only puffy
red stars known as
red supergiants could end their lives in a supernova.
In the failed supernova of a
red supergiant, the envelope of the
star is ejected and expands, producing a cold,
red transient source surrounding the newly formed black hole, as illustrated by the expanding shell (left to right).
When the cores of certain «
red supergiant»
stars collapse, instead of making supernovae, they may form black holes that simply swallow up the disintegrating
star.
Stars with more than about 10 solar masses, after burning their hydrogen become
red supergiants during their helium - burning phase.
Deneb is tied with Orion's foot
star, Rigel, as the most luminous bright
star in the heavens — a white
supergiant, more dazzling than the famous
red variety.
Counterclockwise from bottom: Researchers have spotted three baby
stars at the center of the Milky Way, discovered a large molecular cloud that they believe will turn into a massive
star, and watched a
red supergiant, Be
Red supergiants are the largest type of
star known, and Betelgeuse, part of the Orion constellation, is a formidable member of that class.
Researchers from the University of California, Berkeley, reported yesterday at the meeting that Betelgeuse — a
red supergiant that, back in 1921, was the first
star ever to have its size measured — has steadily shrunk in diameter by 15 % over the past 15 years.
By comparing data from IUE before and after the explosion was observed, astronomers identified the progenitor
star — and found that it was a blue, rather than a
red,
supergiant.
Towards the end of their lives, massive
stars expand rapidly and become
red giants or
supergiants, like Betelgeuse in the Orion constellation.
Before 1987, astronomers believed that only
red supergiants would explode as supernovae, but this observation proved that other types of evolved
stars can produce these explosions too.
& Cantiello, M. Evolution of massive
stars with pulsation - driven superwinds during the
red supergiant phase.
«This alters our basic understanding of
red -
supergiant star atmospheres,» explains Lim.
The
red star at the center of the eyeball - like feature is an unusual erupting
supergiant called V838 Monocerotis, located about 20,000 light - years away in the winter constellation Monoceros (the Unicorn).
A highly evolved,
red giant
star, Gacrux is still much smaller than the
red supergiant Betelgeuse, at left.
Jeremy Lim of the Academia Sinica Institute of Astronomy & Astrophysics in Taiwan; Chris Carilli, Anthony Beasley, and Ralph Marson of the National Radio Astronomy Observatory (NRAO) in Socorro, NM; and Stephen White of the University of Maryland studied the
red -
supergiant star Betelgeuse, about 430 light - years away in the constellation Orion.
«This method for propelling the mass outflows of
red giant and
supergiant stars was proposed by Sun Kwok in the same year that Martin Schwarzschild postulated the existence of large convection cells on these
stars,» Lim said.
«The idea that
red -
supergiant stars have enormous convection cells is not new,» noted Marson.
[64]
Supergiant stars often swing between O or B (blue) and K or M (
red).
The observations indicate that iPTF 13dqy was a regular type II supernova; thus, the finding that the probable
red supergiant progenitor of this common explosion ejected material at a highly elevated rate just prior to its demise suggests that pre-supernova instabilities may be common among exploding massive
stars.
Red supergiants are cooler and
redder than dwarfs of the same spectral type, and
stars with particular spectral features such as carbon
stars may be far
redder than any black body.
The sharp «eye» of the Wide Field Camera 3 (WFC3) has captured hundreds of young
star clusters, ancient swarms of globular
star clusters, and hundreds of thousands of individual
stars, mostly blue
supergiants and
red supergiant (Credit: NASA, ESA and the Hubble Heritage Team (STScI / AURA)-RRB-
A highly evolved, orange -
red giant
star, Arcturus is still much smaller than the
red supergiant Betelgeuse, at left.
The sharp «eye» of the Wide Field Camera 3 (WFC3) has captured hundreds of young
star clusters, ancient swarms of globular
star clusters, and hundreds of thousands of individual
stars, mostly blue
supergiants and
red supergiant
A highly evolved, orange -
red giant
star, Aldebaran A is still much smaller than the
red supergiant Betelgeuse, at left.
A highly evolved, orange -
red giant
star, Pollux is still much smaller than the
red supergiant Betelgeuse, at left.
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The
star UY Scuti, visible in the night sky as part of the constellation Scutum, is a
red supergiant that, with a volume nearly five billion times larger than our Sun, is currently the leading candidate for being the largest known
star by radius.